返回
LISA interferometry:: recent developments
DOI:10.1088/0264-9381/23/8/S16.png)
摘要
En 中文
LISA, the Laser Interferometer Space Antenna, will be launched by NASA and ESA in the 2014 timeframe and will be the first gravitational wave observatory for the many fascinating sources at low frequencies (down to 10(-5) Hz). One of the challenges is to perform precision laser interferometry over a distance of 5 million km. This paper describes recent developments in the interferometer design.
Keyword:
GRAVITATIONAL-WAVE MEASUREMENTS
LASER FREQUENCY STABILIZATION
ESA CORNERSTONE MISSION
SPACE ANTENNA
PHASE-LOCKING
ARM-LOCKING
PROGRESS
DELAY
AI总结
对已上传原文的论文进行重点信息的提取,主要内容包括:简要概述、研究摘要、背景介绍、关键亮点、图文解析、展望与总结。
期刊
IF:
3.7
论文数:
1.3W
被引数:
3.0W
机构
暂无机构信息
引用论文
LISA - Astudy of the ESA cornerstone mission for observing gravitational waves
ACTA ASTRONAUTICA
IF3.4

